RMS Images are meant to represent the root-mean-square deviation from the mean (rmsd) appropriate to measure the noise level in a Gaussian distribution.

maximum 6.7898e-04 Jy/beam
minimum 1.1442e-04 Jy/beam
mean 1.8643e-04 Jy/beam
median 1.3926e-04 Jy/beam
sigma 9.5323e-05 Jy/beam
MAD rms 1.4922e-05 Jy/beam

RMS images

VLASS2.1.sb38694041.eb38838729.59146.565794803246_split.ms

VLASS2.1.ql.T03t19.J122023_283000.10.2048.v1.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T03t19.J122023-283000_P73261v1_2020_10_24T18_49_50.831/working/VLASS2.1.sb38694041.eb38838729.59146.565794803246_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T03t19.J122023-283000_P73261v1_2020_10_24T18_49_50.831/working
Start time
2020-11-18 15:19:15.715
End
2020-11-18 15:20:37.153
Duration
0:01:21.439
Note, WebLog generation is not included in the time.

CASA logs for stage 6